He, Ne, and Ar from the solar wind and solar energetic particles in lunar ilmenites and pyroxenes

Author:

Benkert Jean-Paul,Baur Heinrich,Signer Peter,Wieler Rainer

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference51 articles.

1. Abundances of the elements: meteoritic and solar;Anders;Geochim. Cosmochim. Acta,1989

2. Cosmic ray exposure ages of Apollo 17 samples and the age of Tycho;Arvidson;Proc. Lunar Sci. Conf. 7th,1976

3. Model calculations of solar wind and SEP neon isotopic distributions in lunar regolith grains, (abstract);Becker;Lunar Planet. Sci.,1990

4. Long-term changes in solar wind elemental and isotopic ratios: a comparison of two lunar ilmenites of different antiquities;Becker;Geochim. Cosmochim. Acta,1989

5. Composition of solar wind noble gases released by surface oxidation of a metal separate from the Weston meteorite;Becker;Earth Planet. Sci. Lett.,1991

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